Stereo Pairs 
An explanation of stereo pairs and their use (PDF)  

Planned stereo pairs have suitable stereo convergence angles and illumination by design. In addition to planned stereo pairs, the Pairendipity software can identify overlapping HiRISE images that are serendipitously suitable for stereo processing and find stereo pairs within the CTX dataset.

Planned HiRISE stereo pairs are listed in the “Stereo Pair List (CSV)” link below. Since this list is based on produced stereo anaglyphs it also contains a few serendipitous pairs that underwent special processing. Most serendipitous HiRISE stereo pairs are listed in the “Pairendipity Stereo” link, while CTX stereo pairs are listed in “Pairendipity CTX Stereo”.

Images taken close together in time minimize illumination and frost differences and are especially useful (see the Delta-Days column in the Pairendipity files or difference the orbit numbers in the image IDs in the Stereo Pair List file). Stereo pairs with both images planned within the same 14-day (168-orbit) operations cycle are known as SPORCs.

Layers on Northern Rim of Hellas Basin:   ESP_024408_1500   ESP_031911_1500   (Interval in Earth days: 585)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-29.4

70.8

-7.5

5.233

51.0

33.6

Large Impact Crater Northwest of Lyot Crater:   ESP_024370_2445   ESP_024291_2445   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
63.94

10.5

13.3

-2.50

62.1

64.0

Dune Composition:   ESP_025042_1375   ESP_024976_1375   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-42.3

42.0

0.35

18.39

69.4

67.5

Meanders and Tributaries in Ridge Form in the Zephyria Region:   ESP_024484_1750   ESP_024985_1750   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.09

151.

4.43

19.16

38.5

43.0

Lava Coating, Flood-Carved Kasei Valles:   ESP_024202_2010   ESP_024703_2010   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
20.84

287.

-2.9

19.15

38.0

35.7

The Eastern Floor of Aram Chaos:   ESP_024266_1830   ESP_023910_1830   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
3.112

340.

24.6

9.188

33.0

32.9

Proctor Crater Dune Changes:   ESP_024291_1320   ESP_024370_1320   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-47.6

30.3

-29.

-0.98

63.3

62.9

Harmakhis Vallis Terrain Sample:   ESP_024249_1405   ESP_024394_1405   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-39.2

92.0

-1.1

16.31

54.7

56.2

Alluvial Fans and Hanging Valley Morphology in Kasei Valles:   ESP_024215_2030   ESP_024637_2030   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
22.69

291.

8.75

-2.72

37.8

37.9

Mantle Removal around Gully Fan:   ESP_024027_1345   ESP_024304_1345   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-45.4

33.9

-5.9

-21.5

55.7

61.3


  


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